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  2. Bremsstrahlung - Wikipedia

    en.wikipedia.org/wiki/Bremsstrahlung

    Bremsstrahlung produced by a high-energy electron deflected in the electric field of an atomic nucleus. In particle physics, bremsstrahlung / ˈ b r ɛ m ʃ t r ɑː l ə ŋ / [1] (German pronunciation: [ˈbʁɛms.ʃtʁaːlʊŋ] ⓘ; from German bremsen 'to brake' and Strahlung 'radiation') is electromagnetic radiation produced by the deceleration of a charged particle when deflected by ...

  3. Kramers' opacity law - Wikipedia

    en.wikipedia.org/wiki/Kramers'_opacity_law

    Kramers' opacity law describes the opacity of a medium in terms of the ambient density and temperature, assuming that the opacity is dominated by bound-free absorption (the absorption of light during ionization of a bound electron) or free-free absorption (the absorption of light when scattering a free ion, also called bremsstrahlung). [1]

  4. Beamstrahlung - Wikipedia

    en.wikipedia.org/wiki/Beamstrahlung

    Beamstrahlung (from beam + bremsstrahlung) is the radiation from one beam of charged particles in storage rings, linear or circular colliders, namely the synchrotron radiation emitted due to the electromagnetic field of the opposing beam. [1] [2] Coined by J. Rees in 1978. [3]

  5. Continuum mechanics - Wikipedia

    en.wikipedia.org/wiki/Continuum_mechanics

    Continuum mechanics is a branch of mechanics that deals with the deformation of and transmission of forces through materials modeled as a continuous medium (also called a continuum) rather than as discrete particles. Continuum mechanics deals with deformable bodies, as opposed to rigid bodies. A continuum model assumes that the substance of the ...

  6. Kramers' law - Wikipedia

    en.wikipedia.org/wiki/Kramers'_law

    Kramers' law is a formula for the spectral distribution of X-rays produced by an electron hitting a solid target. The formula concerns only bremsstrahlung radiation, not the element specific characteristic radiation.

  7. Solar radio emission - Wikipedia

    en.wikipedia.org/wiki/Solar_radio_emission

    The storm continuum can last from hours to days and may transition into an ordinary Type I noise storm in long-duration events. [6] Both flare and storm continuum Type IV bursts are attributed to plasma emission, but the storm continuum exhibits much larger degrees of circular polarization for reasons that are not fully known. [16]

  8. Synchrotron radiation - Wikipedia

    en.wikipedia.org/wiki/Synchrotron_radiation

    Synchrotron radiation is similar to bremsstrahlung radiation, which is emitted by a charged particle when the acceleration is parallel to the direction of motion. The general term for radiation emitted by particles in a magnetic field is gyromagnetic radiation , for which synchrotron radiation is the ultra-relativistic special case.

  9. Bethe formula - Wikipedia

    en.wikipedia.org/wiki/Bethe_formula

    For electrons the energy loss is slightly different due to their small mass (requiring relativistic corrections) and their indistinguishability, and since they suffer much larger losses by Bremsstrahlung, terms must be added to account for this. Fast charged particles moving through matter interact with the electrons of atoms in the material.